MEGARA Pipeline

Overview

MEGARA (Multi-Espectrografo en GTC de Alta Resolucion para Astronomia) is an optical IFU and multi-object spectrograph on the 10.4 m Gran Telescopio Canarias (GTC). It features a hexagonal fiber bundle of 623 fibers covering a 12.5” x 11.3” field of view, with fiber core diameter of 0.62”.

3DCubeGen provides a complete pipeline for MEGARA that integrates the numina / megaradrp Data Reduction Pipeline (DRP) with the kernel interpolation cube reconstruction.

CLI Entry Point

The MEGARA pipeline is accessed via the pipemegara command:

pipemegara <command> [options]

Two commands are available:

Command

Purpose

rundrp

Manual step-by-step DRP execution + cube reconstruction

runfulldrp

Fully automated pipeline: sort observations, reduce calibrations, calibrate science data, and reconstruct cubes

rundrp

The rundrp command runs the MEGARA DRP reduction steps individually and then reconstructs a data cube. It requires the numina framework to be installed and the MEGARA DRP configuration files (obsresult-*.yaml, requirements-*.yaml) to be present in the working directory.

The reduction follows this calibration chain:

  1. Bias – master bias creation

  2. Traces – fiber trace identification

  3. Wavelength calibration – arc lamp wavelength solution

  4. Fiber flat – fiber-to-fiber response correction

  5. Standard star – spectrophotometric calibration

  6. Science – final science frame reduction + cube reconstruction

pipemegara rundrp --redux_dir /path/to/data --stdar_t HD12345 --vph LR-R

Key options:

Option

Default

Description

-o, --out_path

out_cubes

Output directory for the final cube

-r, --redux_dir

''

Path to the working directory with raw data

-s, --sigm_s

0.35

Smoothing kernel size (arcsec)

-p, --pix_s

0.0

Spaxel size (0 = same as sigm_s)

-a, --alph_s

2.0

Kernel shape factor

-m, --stdar_t

Name of the spectrophotometric standard star

-y, --vph

LR-R

VPH grating name (e.g., LR-B, LR-R, LR-Z, MR-R, HR-R)

-u, --aper_std

4.0

Aperture radius for spectrophotometric calibration (arcsec)

-b, --basename

megCube-NAME.fits

Output cube basename template

runfulldrp

The runfulldrp command automates the entire reduction workflow. It:

  1. Sorts observation files by type (bias, arc, flat, standard, science)

  2. Generates the DRP configuration files automatically

  3. Runs all calibration steps

  4. Performs spectrophotometric calibration iteratively

  5. Reconstructs the final data cube

  6. Extracts a 1D spectrum

It can be driven by CLI options or by a YAML configuration file.

pipemegara runfulldrp -c config_runfulldrp.yml

# Or with CLI options:
pipemegara runfulldrp --run_name GTC5-24AMEX --run_number 0001 \
    --obrun_path /path/to/raw --redux_path /path/to/redux \
    --out_path /path/to/output

Key additional options:

Option

Default

Description

-t, --run_name

GTC5-24AMEX

Name of the GTC observation run

-g, --run_number

0001

Observation block number (string format)

-m, --obrun_path

''

Path to the raw observation data

-r, --redux_path

''

Working directory for intermediate reduction products

-c, --config_file

''

Path to YAML config file (overrides CLI options)

-e, --forcear

False

Force use of ThAr arc lamp for wavelength calibration

Configuration File

The runfulldrp command accepts a YAML configuration file. A template is provided at CubeGen/megaratools/configfiles/config_runfulldrp.yml:

---
run_drp:
  - pipe_type: FULL
    run_name: GTC5-24AMEX
    run_number: '0001'
    out_path: out_cubes
    redux_ver: 1.1.1.dev0
    redux_path: ''
    obrun_path: ''
    sigm_s: 0.35
    pix_s: 0.0
    alph_s: 2.0
    flu16: True
    name: None
    basename: megCube-NAME.fits
    fac_sizey: 1.0
    fac_sizex: 1.0
    aper_std: 4.0
    forcear: False

Differences from LVM

While MEGARA uses the same core kernel interpolation algorithm, several defaults and behaviors differ:

Aspect

MEGARA

LVM

Default sigm_s

0.35” (sub-arcsecond)

32.2” (wide fibers)

pix_s when 0

Same as sigm_s

0.75 * sigm_s

Fiber geometry

623 fibers, hexagonal, 0.62” core

~1800 science fibers, 35.3” pitch

VPH selection

Multiple gratings (LR-B/R/Z, MR, HR)

N/A (fixed spectral range)

Spectrophotometric cal

Built into pipeline (iterative)

External (pre-calibrated SFrames)

DRP integration

Runs numina + megaradrp

Reads pre-reduced RSS frames